The 18S ribosomal RNA sequence of the sea anemone <i>Ammonia sulcata</i> and its evolutionary position among other eukaryotes

Evolutionary trees based on partial small ribosomal subunit RNA sequences of 22 metazoa species have been published [(1988) Science 239, 748-753]. In these trees, cnidarians (Radiata) seemed to have evolved independently from the Bilateria, which is in contradiction with the general evolutionary view. In order to further investigate this problem, the complete srRNA sequence of the sea anemone Ammonia sulcata was determined and evolutionary trees were constructed using a matrix optimization method. In the tree thus obtained the sea anemone and Bilateria together form a monophyletic cluster, with the sea anemone forming the first line of descent of the metazoan group

Equivalence of Kinetic Theories of Bose-Einstein Condensation

We discuss the equivalence of two non-equilibrium kinetic theories that describe the evolution of a dilute, Bose-Einstein condensed atomic gas in a harmonic trap. The second-order kinetic equations of Walser et al. [PRA 63, 013607 (2001)] reduce to the Gross-Pitaevskii equation and the quantum Boltzmann equation in the low and high temperature limits, respectively. These kinetic equations can thus describe the system in equilibrium (finite temperature) as well as in non-equilibrium (real time). We have found this theory to be equivalent to the non-equilibrium Green's function approach originally proposed by Kadanoff and Baym and more recently applied to inhomogeneous trapped systems by M. Imamovi\'c-Tomasovi\'c and A. Griffin [arXiv:cond-mat/9911402].Comment: REVTeX3, 6 pages, 2 eps figures, published version, minor change

Oximetry and Glucose Sensors A SMART SENSOR FOR BIOMEDICAL APPLICATIONS

Abstract Monolithic smart sensors for the voltammetric measurement of glucose or oxygen concentrations have been developed. Each smart sensor consists of a planar voltammetric sensor, a CMOS interface circuit and temperature sensor. The interface circuit and the temperature sensor are realised in a standard CMOS process. The sensor specific layers are added afterwards on the same chip with the CMOS compatible sensor technology developed for this purpose. Two versions of this smart sensor have been realised. The two electrode configuration with a Au working electrode has been implemented for the measurement of p02. The three electrode configuration with a Pt working electrode can measure glucose when an additional glucose oxidase membrane is applied on the electrodes. The interface circuit can apply voltages from +lV to -lV to the sensor and can handle sensor current ranges from 30 nA full scale to 1 pA full scale with a +/-2.5 V supply voltage. The temperature sensor has a sensitivity of 154 pV/K. The total dimensions of this smart sensor are 0.75 mm by 5 mm

White Dwarf - Red Dwarf Systems Resolved with the Hubble Space Telescope: I. First Results

First results are presented for a Hubble Space Telescope Advanced Camera for Surveys snapshot study of white dwarfs with likely red dwarf companions. Of 48 targets observed and analyzed so far, 27 are totally or partially resolved into two or more components, while an additional 15 systems are almost certainly unresolved binaries. These results provide the first direct empirical evidence for a bimodal distribution of orbital separations among binary systems containing at least one white dwarf.Comment: 46 pages, 3 figures, 5 tables, accepted to ApJ. Full-resolution images available upon request. A few table entries correcte

Magnetic susceptibility of EuTe/PbTe Heisenberg superlattices: experimental and theoretical studies

We report results on the temperature dependence of the susceptibilities of a set of MBE-grown short-period EuTe/PbTe antiferromagnetic superlattices having different EuTe layer thicknesses. In-plane and orthogonal susceptibilities have been measured and display a strong anisotropy at low temperature, confirming the occurrence of a magnetic phase transition in the thicker samples, as seen also in neutron diffraction studies. We suggest that dipolar interactions stabilize antiferromagnetic long-range order in an otherwise isotropic system and we present numerical and analytical results for the low-temperature orthogonal susceptibility.Comment: 30 pages, 8 ps figures, RevTe

Near-infrared spectro-interferometry of three OH/IR Stars with the VLTI/AMBER instrument

We investigate the molecular and dusty environment of OH/IR stars in order to characterize the mass-loss process during the tip-AGB superwind phase. Employing the AMBER instrument at the VLT Interferometer we obtained near-infrared H- and K-band spectro-interferometric observations of the three OH/IR stars IRAS 13479-5436, IRAS 14086-6907 and IRAS 17020-5254 with a spectral resolution of about 35. We use a two-component geometrical model, consisting of a uniform disk and a Gaussian disk, to obtain characteristic angular sizes of the central stellar sources and their dust envelopes, as well as the flux ratios between these components. Angular uniform disk diameters of the three central components of the objects above have values between 3.2 mas and 5.4 mas. For their dust envelopes, we find FWHM values between 17.1 mas and 25.2 mas. According to distance estimates from the literature, the central stellar components have radii between 900 R_sun and 1400 R_sun, while their dust envelopes reach FWHM values between 9000 R_sun and 13000 R_sun. The visibility functions of all three sources exhibit wavelength variations that resemble those of earlier VLTI/AMBER observations of semi-regular and Mira variable AGB stars. These are interpreted as characteristic of atmospheric molecular layers lying above the photosphere. We also find that the dust envelopes have a clearly larger optical depth than those known for Mira stars. We interpret this as an expected result of the "superwind" phase, the final 10 000 to 30 000 years of AGB-evolution, when the mass-loss rate increases by a factor of 10-100. By their different optical depths, the three dust shells studied here may represent different stages of the "superwind" and different initial masses.Comment: 5 pages, 6 figures, accepted for publication in Astronomy and Astrophysic